This book sets forth and builds upon the fundamentals of the dynamics of
natural systems in formulating the problem presented by Jacobi in his
famous lecture series "Vorlesungen tiber Dynamik" (Jacobi, 1884). In the
dynamics of systems described by models of discrete and continuous
media, the many-body problem is usually solved in some approximation, or
the behaviour of the medium is studied at each point of the space it
occupies. Such an approach requires the system of equations of motion to
be written in terms of space co-ordinates and velocities, in which case
the requirements of an internal observer for a detailed description of
the processes are satisfied. In the dynamics discussed here we study the
time behaviour of the fundamental integral characteristics of the
physical system, i. e. the Jacobi function (moment of inertia) and
energy (potential, kinetic and total), which are functions of mass
density distribution, and the structure of a system. This approach
satisfies the requirements of an external observer. It is designed to
solve the problem of global dynamics and the evolution of natural
systems in which the motion of the system's individual elements written
in space co-ordinates and velocities is of no interest. It is important
to note that an integral approach is made to internal and external
interactions of a system which results in radiation and absorption of
energy. This effect constitutes the basic physical content of global
dynamics and the evolution of natural systems.